微硅加速度传感器的动态特性补偿方法研究

提出了一种用以扩展加速度传感器使用频率范围的动态特性补偿方法,其基本原理是根据加速度传感器的输入输出传递函数,构造出一个基于硬件的补偿网络,这个补偿网络的传递函数的零极点分别与加速度传感器的传递函数的极零点相抵消,从而使由加速度传感器输出的信号经过补偿环节后其动态特性得到补偿,扩展了加速度传感器的使用频带,同时并不要求加速度传感器处于临界阻尼状态。     

Hard X-ray observations of the Crab Pulsar

The Crab was observed in a balloon flight from Palestine/Texas on 9/28/81 at hard X-ray energies (20–200 keV). The light curve is significantly sharper than reported previously for this energy range. The pulse-averaged as well as the interpulse spectra show breaks in our energy-range. The variation of spectral index across the pulse has an amplitude similar to that found at lower energies by OSO-8 and larger than reported by HEAO-1 A4 at hard X-rays. For a sharp emission line at 77 keV a 99% upper limit of 1.0*10⁻³ photons/ cm² sec can be placed, a factor of 4 lower than line fluxes reported previously. Pulse-shape fits to the optical, X-ray, hard X-ray and gamma ray light-curves reveal a consistent picture of the origin of the interpulse and off-pulse emission, the breaks in the spectra and the variation of spectral index, providing arguments against a thermal component and also a polar cap emission model for NP0532.     

高中低能电子联合辐照电介质薄膜充放电效应

高能(350KeV)-中能(18—30KeV可调)-低能(4—5KeV可调)电子联合辐照聚酯薄膜和特氟隆薄膜,得到与中能电子辐照、高-中能电子联合辐照以及中-低能电子联合辐照不同的结果。实验结果表明,高能电子能诱发电介质薄膜充放电。特氟隆薄膜的三能电子联合辐照实验结果与Coakley和Treadaway的1-100keVdN/dE∝E~(-2)谱电子辐照实验结果以及NASCAP计算机模拟结果符合。得出结论,三能电子联合辐照可较为完善地模拟静止卫星电介质的充放电效应。论证了选用三种能量电子的充分性和必要性。推断出,如果在星食期遇到象1979年4月24日磁层亚暴事件,则静止卫星表面某些电介质局部电位有可能超过SCATHA卫星近期数据给出的和NASCAP计算的-2—-4KV,而且会出现大的放电。     

Dosimetric mapping inside BIORACK

The experiment was flown in different locations inside BIORACK on the D1 mission. It contained different plastic detectors (cellulose nitrate, Lexan, and CR 39) and emulsions to measure the high LET components of the radiation environment. For low LET measurements thermoluminescence dosimeters (L iF) were used. The paper gives data about total dose, charge, energy, and LET spectra so far obtained. These data are compared with data of previous spaceflights.     

Embryogenesis and organogenesis of Carausius morosus under spaceflight conditions

The influence of cosmic radiation and/or microgravity on insect development was studied during the 7 day German Spacelab Mission D1. Eggs of Carausius morosus of five stages differing in sensitivity to radiation and in capacity to regeneration were allowed to continue their development in the BIORACK 22°C incubator, either at microgravity conditions or on the 1 g reference centrifuge. Using the Biostack concept - eggs in monolayers were sandwiched between visual track detectors - and the 1 g reference centrifuge, we were able to separate radiation effects from microgravity effects and also from combined effects of these two factors in space. After retrieval, hatching rates, growth kinetics and anomaly frequencies were determined in the different test samples. The early stages of development turned out to be highly sensitive to single hits of cosmic ray particles as well as to the temporary exposure to microgravity during their development. In some cases, the combined action of radiation and microgravity even amplified the effects exerted by the single parameters of space. Hits by single HZE particles caused early effects, such as body anomalies, as well as late effects, such as retarded growth after hatching. Microgravity exposure lead to a reduced hatching rate. A synergistic action of HZE particle hits and microgravity was established in the unexpectedly high frequency of anomal larvae. However, it cannot be excluded, that cosmic background radiation or low LET HZE particles are also causally involved in damage observed in the microgravity samples.     

一种模拟CCD星图的方法

星识别算法在空间飞行器自主姿确定系统中是不可缺少的。同时将ＣＣＤ所拍摄的星图作为算法的输入,无论是软件调试还是地面试验,抑或是对各种算法的评估,也是必不可缺少。     

结合小波变换的Jacquin分形图像编码

提出了一种将分形与小波变换紧密结合起来的图像压缩方法;改进了目前虽简单易行,但编码时间过长的分形图像编码,而且Domain块的采样方式也存在缺陷。针对这些问题,利用小波分解的特性构造了一种基于小波分解的分形图像编码算法;对输入图像进行小波变换,将变换后的低频部分作为Jacquin分形编码方法的搜索区域。实验表明重构图像的质量得到了较大的提高。     

Correction to: Determining the Relative Cratering Ages of Regions of Psyche’s Surface

Space Science Reviews - Analysis of Homestake, Gallex and GNO measurements reveals evidence of variability of presumed solar-neutrino-flux measurements. Analysis of Super-Kamiokande neutrino...     

助推器喷口火焰温度测量

火焰温度测量是一个复杂而困难的问题。接触式测温传感器在很多情况下并不适用。固体燃料助推器火焰中有大量固体粒子,这些固体粒子运动速度又很高,采用接触式测温传感器测量这种火焰温度问题较多。介绍用四支小型不调焦光电高温计从不同角度测量固体燃料助推器喷口火焰温度的试验装置和试验结果,并对小型不调焦光电高温计的基本原理、结构、性能作了简单介绍。     

烧蚀模型表面温度分布测量

介绍了一维表面温度分布的非接触测量仪器——扫描光电高温计的基本原理、结构、性能以及实用情况。扫描光电高温计的研制成功,使烧蚀模型表面温度测量从点温度测量拓展到一维温度分布测量,解决了突缩管壁面热分布的研究问题,测量了各种材料烧蚀模型驻点区温度分布曲线和不同材料平板模型在烧蚀试验中沿射流流向和径向的温度分布,并利用弓型导管装置对不同开槽型的石墨平板模型和喷有氧化锆隔热涂层的平板试件进行了温度场的测量。同时,还介绍了偏转装置与扫描光电高温计配合使用,一次开车试验可以测量不同位置上一维温度分布。